Mapping Titan's HCN in the far infra-red: implications for photochemistry.
Observations of Titan's far infra-red spectra by the Cassini orbiter's Composite InfraRed Spectrometer have been used to determine the latitude distribution of HCN at 1 mbar by fitting the HCN and CO rotational lines in the 18-60 cm(-1) (160-550 microm) spectral range. Results confirm the...
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| Aineistotyyppi: | Conference item |
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2010
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